卡拉天体二折射玻璃和熔融硅酸盐玻璃的比较特性

A. Zubov, T. Shumilova, S. Isaenko
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引用次数: 0

摘要

研究对象为卡拉火山脉状熔体撞击形成的硅酸盐玻璃和熔融硅酸盐玻璃。获得了两种形成机理完全不同的玻璃的微观和光谱特征,从而可以比较它们的结构特征。我们发现,来自Kara astrobleme的高压/高温脉体的硅酸盐弹射玻璃和熔融冲击玻璃具有相似的结构特征——高度聚合,存在四元和多元SiO4环,这是所有玻璃的特征,即SiO2成分。偏光玻璃的特点是三元SiO4环的持续存在;熔融玻璃的特点是没有这种特征,这是由更极端的熔融玻璃条件决定的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparative characteristics of diaplectic and melt silicate glasses of the Kara astrobleme
The objects of study are diaplectic and melt silicate glasses from vein melt impactites of the Kara astrobleme. Microscopic and spectroscopic characteristics of two glasses with fundamentally different formation mechanisms were obtained, which allowed comparing their structural features. We found that silicate diaplectic and melt impact glasses from high-pressure/high-temperature vein bodies of the Kara astrobleme were characterized by similar structural features — a high degree of polymerization, the presence of four-membered and polymembered SiO4 rings, which was characteristic of all glasses were the SiO2 composition. Diaplectic glasses are characterized by the constant presence of three-membered SiO4 rings; melt glasses were characterized by the absence of this feature, which was determined by more extreme conditions for the glass from melt.
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